Instability of compact stars with a nonminimal scalar-derivative coupling
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Publication:5025248
DOI10.1088/1475-7516/2021/01/008zbMath1484.85014arXiv2008.13350OpenAlexW3120546323MaRDI QIDQ5025248
Ryotaro Kase, Shinji Tsujikawa
Publication date: 1 February 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2008.13350
Bifurcations and instability for nonlinear problems in mechanics (70K50) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Galactic and stellar structure (85A15) Stability and instability of geophysical and astrophysical flows (76E20)
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Cites Work
- Variational aspects of relativistic field theories, with application to perfect fluids
- Structure of neutron stars in \(R\)-squared gravity
- Event horizon in static scalar-vacuum space-times
- Exact black hole solutions in shift symmetric scalar-tensor theories
- Generalized G-Inflation: --Inflation with the Most General Second-Order Field Equations--
- Stability of a Schwarzschild Singularity
- DYNAMICS OF DARK ENERGY
- Slowly rotating anisotropic neutron stars in general relativity and scalar–tensor theory
- Action functionals for relativistic perfect fluids
- Analytical representations of unified equations of state of neutron-star matter
- A no-hair theorem for stars in Horndeski theories
- Asymptotically flat black holes in Horndeski theory and beyond
- Scaling solutions and weak gravity in dark energy with energy and momentum couplings
- Dark energy in Horndeski theories after GW170817: A review
- Neutron stars inf(R) gravity and scalar-tensor theories
